On the theory of large amplitude Alfven waves

dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorKlimas, A. J.
dc.contributor.authorBarish, F. D.
dc.date.accessioned2023-11-02T17:57:38Z
dc.date.available2023-11-02T17:57:38Z
dc.date.issued1974-04-01
dc.description.abstractLarge amplitude Alfvenic disturbances of arbitrary spatial shape and polarization are described by MHD equations, without resort to the usual assumption of planarity. However, because of their nonplanar nature, the direction of propagation of these disturbances cannot, in general, be determined by looking for minima in a variance matrix constructed from observed field fluctuations. When such minima exist, one is observing that subset of interplanetary Alfven waves that is essentially planar.en
dc.description.urihttps://ntrs.nasa.gov/citations/19740014712en
dc.format.extent9 pagesen
dc.genrejournal articlesen
dc.genrepreprintsen
dc.identifierdoi:10.13016/m2bdfn-oi5s
dc.identifier.citationGoldstein, M. L., A. J. Klimas, and F. D. Barish. “On the Theory of Large Amplitude Alfven Waves,” April 1, 1974. https://ntrs.nasa.gov/citations/19740014712.en
dc.identifier.urihttp://hdl.handle.net/11603/30498
dc.language.isoenen
dc.publisherNTRSen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis is a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleOn the theory of large amplitude Alfven wavesen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen

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